The spectral energy distribution of powerful starburst galaxies – I. Modelling the radio continuum

Abstract We have acquired radio-continuum data between 70 MHz and 48 GHz for a sample of 19 southern starburst galaxies at moderate redshifts (0.067

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2018-02, Vol.474 (1), p.779-799
Hauptverfasser:	Galvin, T. J., Seymour, N., Marvil, J., Filipović, M. D., Tothill, N. F. H., McDermid, R. M., Hurley-Walker, N., Hancock, P. J., Callingham, J. R., Cook, R. H., Norris, R. P., Bell, M. E., Dwarakanath, K. S., For, B., Gaensler, B. M., Hindson, L., Johnston-Hollitt, M., Kapińska, A. D., Lenc, E., McKinley, B., Morgan, J., Offringa, A. R., Procopio, P., Staveley-Smith, L., Wayth, R. B., Wu, C., Zheng, Q.
Format:	Artikel
Sprache:	eng
Schlagworte:	Absorption Astronomical models Bayesian analysis Bolometers Cosmic rays Curvature Data acquisition Emission Galactic evolution Galaxy distribution High frequencies Power law Radio Spectral energy distribution Star & galaxy formation Star formation Starburst galaxies
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Beschreibung
Zusammenfassung:	Abstract We have acquired radio-continuum data between 70 MHz and 48 GHz for a sample of 19 southern starburst galaxies at moderate redshifts (0.067
ISSN:	0035-8711 1365-2966
DOI:	10.1093/mnras/stx2613